# The Polycyclic Aromatic Hydrocarbon Mass Fraction on a 10 pc scale in   the Magellanic Clouds

**Authors:** Jeremy Chastenet, Karin Sandstrom, I-Da Chiang, Adam Leroy, Dyas, Utomo, Caroline Bot, Karl Gordon, Bruce Draine, Yasuo Fukui, Toshikazu, Onishi, and Kisetsu Tsuge

arXiv: 1904.02705 · 2019-05-15

## TL;DR

This study maps the PAH mass fraction in the Magellanic Clouds, revealing lower PAH abundance in the SMC compared to the LMC and Milky Way, with variations across different gas phases and implications for PAH lifecycle and metallicity.

## Contribution

First detailed spatial mapping of PAH fraction in the Magellanic Clouds using Spitzer and Herschel data, analyzing variations across gas phases and metallicity.

## Key findings

- PAH fraction is lower in the SMC than in the LMC and Milky Way.
- H II regions show a deficit of PAHs compared to other gas phases.
- PAH abundance correlates with metallicity and gas phase conditions.

## Abstract

We present maps of the dust properties in the Small and Large Magellanic Clouds (SMC, LMC) from fitting Spitzer and Herschel observations with the \citet{DL07} dust model. We derive the abundance of the small carbonaceous grain (or polycyclic aromatic hydrocarbon; PAH) component. The global PAH fraction (q_pah, the fraction of the dust mass in the form of PAHs) is smaller in the SMC (1.0$^{+0.3}_{-0.3}$%) than in the LMC (3.3$^{+1.4}_{-1.3}$%). We measure the PAH fraction in different gas phases (H II regions, ionized gas outside of H II regions, molecular gas, and diffuse neutral gas). H II regions appear as distinctive holes in the spatial distribution of the PAH fraction. In both galaxies, the PAH fraction in the diffuse neutral medium is higher than in the ionized gas, but similar to the molecular gas. Even at equal radiation field intensity, the PAH fraction is lower in the ionized gas than in the diffuse neutral gas. We investigate the PAH life-cycle as a function of metallicity between the two galaxies. The PAH fraction in the diffuse neutral medium of the LMC is similar to that of the Milky Way ($\sim4.6$%), while it is significantly lower in the SMC. Plausible explanations for the higher PAH fraction in the diffuse neutral medium of the LMC compared to the SMC include: a more effective PAH production by fragmentation of large grains at higher metallicity, and/or the growth of PAHs in molecular gas.

## Full text

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## Figures

12 figures with captions in the complete paper: https://tomesphere.com/paper/1904.02705/full.md

## References

108 references — full list in the complete paper: https://tomesphere.com/paper/1904.02705/full.md

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Source: https://tomesphere.com/paper/1904.02705